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Fig. 8


[Sr/Zr], [La/Ce], [Nd/Sm], and [Eu/Ba] compared to age. Only stars with age uncertainties less than 3 Gyr are plotted. The black line in each plot represents the best fit. The errors on the ages are taken from Bensby et al. (2014). The average error on the abundance ratio is indicated in the lower left part of each plot.

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